Thermonuclear Reaction Rates for Solar Neutrino Processes
Using the formalism for the effective cross-section factor Seff we calculate the thermonuclear reaction rates and neutrino fluxes for the pp-chain processes. We adopt the recent LUNA experimental data for the nuclear cross-section S-factor and we compute improved and updated solar neutrino fluxes wh...
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Published in | AIP conference proceedings Vol. 972; no. 1; pp. 558 - 561 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
United States
01.01.2008
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Subjects | |
Online Access | Get full text |
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Summary: | Using the formalism for the effective cross-section factor Seff we calculate the thermonuclear reaction rates and neutrino fluxes for the pp-chain processes. We adopt the recent LUNA experimental data for the nuclear cross-section S-factor and we compute improved and updated solar neutrino fluxes which we compare with those previously obtained. |
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Bibliography: | SourceType-Scholarly Journals-2 ObjectType-Feature-2 ObjectType-Conference Paper-1 content type line 23 SourceType-Conference Papers & Proceedings-1 ObjectType-Article-3 |
ISBN: | 9780735404908 0735404909 |
ISSN: | 0094-243X 1551-7616 |
DOI: | 10.1063/1.2870466 |